Open Access
Table B.1.
Nuisance parameters for the photometric (top) and spectroscopic (bottom) surveys. In the spectroscopic survey, the Q-bias and the velocity dispersion parameters are only used in the fully non-linear realistic scenario.
| Photometric survey | ||
|---|---|---|
| Parameter | Symbol | Value |
| Amplitude of IA | 𝒜IA | 1.72 |
| Power-law evolution of IA | ηIA | -0.41 |
| Luminosity dependence of IA | βIA | 2.17 |
| Constant rescaling of IA | 𝒞IA | 0.0134 (fixed) |
| Linear galaxy bias | bi = 1...10 | [1.099773, 1.220246, 1.272399, 1.316624, 1.358124, |
| 1.399821, 1.444645, 1.496496, 1.565248, 1.742986] | ||
| Spectroscopic survey | ||
| Parameter | Symbol | Value |
| Linear galaxy bias | bi = 1...4 | [1.461480, 1.606095, 1.746479, 1.898866] |
| Non-Poissonian shot-noise contribution | Pshot, i = 1..4 | 0 |
| Q-bias denominator | A1 | 0.02 |
| Q-bias numerator | A2 | -2.0 |
| Pairwise velocity dispersion (cosmology dependent) | σp, i = 1...4 | [4.923, 4.629, 4.345, 4.017] |
| Velocity dispersion (cosmology and angle dependent) | σv, i = 1...4 | [5.349, 4.904, 4.522, 4.117] |
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